Posterior density distributions for the retrieved exoplanet parameters (columns) for the different epochs (rows) and cloud coverages. We follow the color-coding listed in Table 1 to differentiate the different scenarios. The vertical, solid lines mark the true values for each parameter. The dotted lines in the R_pl and M_pl plots indicate the assumed Gaussian priors. For P₀ and T₀ we assume broad, flat priors, which are not plotted.